The effects of spatial resolution on Integral Field Spectrograph surveys at different redshifts. The CALIFA perspective
Over the past decade, 3D optical spectroscopy has become the preferred tool for understanding the properties of galaxies and is now increasingly used to carry out galaxy surveys. Low redshift surveys include SAURON, DiskMass, ATLAS3D, PINGS and VENGA. At redshifts above 0.7, surveys such as MASSIV,...
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ftdatacite:10.48550/arxiv.1311.3941 2023-05-15T18:12:35+02:00 The effects of spatial resolution on Integral Field Spectrograph surveys at different redshifts. The CALIFA perspective Mast, D. Rosales-Ortega, F. F. Sanchez, S. F. Vílchez, J. M. Iglesias-Paramo, J. Walcher, C. J. Husemann, B. Marquez, I. Marino, R. A. Kennicutt, R. C. Monreal-Ibero, A. Galbany, L. de Lorenzo-Caceres, A. Mendez-Abreu, J. Kehrig, C. del Olmo, A. Relano, M. Wisotzki, L. Marmol-Queralto, E. Bekeraite, S. Papaderos, P. Wild, V. Aguerri, J. A. L. Falcon-Barroso, J. Bomans, D. J. Ziegler, B. García-Lorenzo, B. Bland-Hawthorn, J. Lopez-Sanchez, A. R. van de Ven, G. 2013 https://dx.doi.org/10.48550/arxiv.1311.3941 https://arxiv.org/abs/1311.3941 unknown arXiv https://dx.doi.org/10.1051/0004-6361/201321789 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences article-journal Article ScholarlyArticle Text 2013 ftdatacite https://doi.org/10.48550/arxiv.1311.3941 https://doi.org/10.1051/0004-6361/201321789 2022-04-01T13:13:00Z Over the past decade, 3D optical spectroscopy has become the preferred tool for understanding the properties of galaxies and is now increasingly used to carry out galaxy surveys. Low redshift surveys include SAURON, DiskMass, ATLAS3D, PINGS and VENGA. At redshifts above 0.7, surveys such as MASSIV, SINS, GLACE, and IMAGES have targeted the most luminous galaxies to study mainly their kinematic properties. The on-going CALIFA survey ($z\sim0.02$) is the first of a series of upcoming Integral Field Spectroscopy (IFS) surveys with large samples representative of the entire population of galaxies. Others include SAMI and MaNGA at lower redshift and the upcoming KMOS surveys at higher redshift. Given the importance of spatial scales in IFS surveys, the study of the effects of spatial resolution on the recovered parameters becomes important. We explore the capability of the CALIFA survey and a hypothetical higher redshift survey to reproduce the properties of a sample of objects observed with better spatial resolution at lower redshift. Using a sample of PINGS galaxies, we simulate observations at different redshifts. We then study the behaviour of different parameters as the spatial resolution degrades with increasing redshift. : 20 pages, 16 figures. Accepted for publication in A&A Text sami DataCite Metadata Store (German National Library of Science and Technology) |
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DataCite Metadata Store (German National Library of Science and Technology) |
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Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
spellingShingle |
Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences Mast, D. Rosales-Ortega, F. F. Sanchez, S. F. Vílchez, J. M. Iglesias-Paramo, J. Walcher, C. J. Husemann, B. Marquez, I. Marino, R. A. Kennicutt, R. C. Monreal-Ibero, A. Galbany, L. de Lorenzo-Caceres, A. Mendez-Abreu, J. Kehrig, C. del Olmo, A. Relano, M. Wisotzki, L. Marmol-Queralto, E. Bekeraite, S. Papaderos, P. Wild, V. Aguerri, J. A. L. Falcon-Barroso, J. Bomans, D. J. Ziegler, B. García-Lorenzo, B. Bland-Hawthorn, J. Lopez-Sanchez, A. R. van de Ven, G. The effects of spatial resolution on Integral Field Spectrograph surveys at different redshifts. The CALIFA perspective |
topic_facet |
Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
description |
Over the past decade, 3D optical spectroscopy has become the preferred tool for understanding the properties of galaxies and is now increasingly used to carry out galaxy surveys. Low redshift surveys include SAURON, DiskMass, ATLAS3D, PINGS and VENGA. At redshifts above 0.7, surveys such as MASSIV, SINS, GLACE, and IMAGES have targeted the most luminous galaxies to study mainly their kinematic properties. The on-going CALIFA survey ($z\sim0.02$) is the first of a series of upcoming Integral Field Spectroscopy (IFS) surveys with large samples representative of the entire population of galaxies. Others include SAMI and MaNGA at lower redshift and the upcoming KMOS surveys at higher redshift. Given the importance of spatial scales in IFS surveys, the study of the effects of spatial resolution on the recovered parameters becomes important. We explore the capability of the CALIFA survey and a hypothetical higher redshift survey to reproduce the properties of a sample of objects observed with better spatial resolution at lower redshift. Using a sample of PINGS galaxies, we simulate observations at different redshifts. We then study the behaviour of different parameters as the spatial resolution degrades with increasing redshift. : 20 pages, 16 figures. Accepted for publication in A&A |
format |
Text |
author |
Mast, D. Rosales-Ortega, F. F. Sanchez, S. F. Vílchez, J. M. Iglesias-Paramo, J. Walcher, C. J. Husemann, B. Marquez, I. Marino, R. A. Kennicutt, R. C. Monreal-Ibero, A. Galbany, L. de Lorenzo-Caceres, A. Mendez-Abreu, J. Kehrig, C. del Olmo, A. Relano, M. Wisotzki, L. Marmol-Queralto, E. Bekeraite, S. Papaderos, P. Wild, V. Aguerri, J. A. L. Falcon-Barroso, J. Bomans, D. J. Ziegler, B. García-Lorenzo, B. Bland-Hawthorn, J. Lopez-Sanchez, A. R. van de Ven, G. |
author_facet |
Mast, D. Rosales-Ortega, F. F. Sanchez, S. F. Vílchez, J. M. Iglesias-Paramo, J. Walcher, C. J. Husemann, B. Marquez, I. Marino, R. A. Kennicutt, R. C. Monreal-Ibero, A. Galbany, L. de Lorenzo-Caceres, A. Mendez-Abreu, J. Kehrig, C. del Olmo, A. Relano, M. Wisotzki, L. Marmol-Queralto, E. Bekeraite, S. Papaderos, P. Wild, V. Aguerri, J. A. L. Falcon-Barroso, J. Bomans, D. J. Ziegler, B. García-Lorenzo, B. Bland-Hawthorn, J. Lopez-Sanchez, A. R. van de Ven, G. |
author_sort |
Mast, D. |
title |
The effects of spatial resolution on Integral Field Spectrograph surveys at different redshifts. The CALIFA perspective |
title_short |
The effects of spatial resolution on Integral Field Spectrograph surveys at different redshifts. The CALIFA perspective |
title_full |
The effects of spatial resolution on Integral Field Spectrograph surveys at different redshifts. The CALIFA perspective |
title_fullStr |
The effects of spatial resolution on Integral Field Spectrograph surveys at different redshifts. The CALIFA perspective |
title_full_unstemmed |
The effects of spatial resolution on Integral Field Spectrograph surveys at different redshifts. The CALIFA perspective |
title_sort |
effects of spatial resolution on integral field spectrograph surveys at different redshifts. the califa perspective |
publisher |
arXiv |
publishDate |
2013 |
url |
https://dx.doi.org/10.48550/arxiv.1311.3941 https://arxiv.org/abs/1311.3941 |
genre |
sami |
genre_facet |
sami |
op_relation |
https://dx.doi.org/10.1051/0004-6361/201321789 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1311.3941 https://doi.org/10.1051/0004-6361/201321789 |
_version_ |
1766185092770693120 |